We combine beam-matched CO-13, CO-12 J = 3 yields 2 and J = 2 yields 1 line data to infer the molecular gas excitation conditions in the central 500 to 1600 pc diameters of a small sample of infrared-bright external galaxies: NGC253, IC342, M 83, Maffei 2, and NGC6946. Additional observations of the J = 1 yields 0 lines of C-18O and CO-13 set limits on the opacity of the CO-13 J = 1 yields 0 line averaged over the central kiloparsec of these spiral galaxies
The correlation between the CO and far infrared luminosities of spiral galaxies is well established....
We present 12CO $J=1$–0 and $J=2$–1 Swedish-ESO Submillimetre Telescope (SEST) observations of the b...
We measure the radial profile of the ^(12)CO(1-0) to H_2 conversion factor (X_(CO)) in NGC 628. The ...
Multi-line studies of CO-12, CO-13, C-18O, HCN, and HCO(+) at 3 mm, 1.3 mm, and 0.8 mm using the Ins...
We estimated physical conditions of molecular gas in the central molecular zone (CMZ) of the Galaxy,...
The CO-to-H2 conversion factor (αCO) is central to measuring the amount and properties of molecular ...
We measure the velocity dispersion, sigma, and surface density, Sigma, of the molecular gas in nearb...
We used the Atacama Pathfinder Experiment (APEX) 12 m telescope to observe the J(KAKc) = 3(03) -> 2(...
Aims. While the search for molecular gas in distant galaxies is based on the detection of submillime...
We present spatial variations of the CO J = 2−1/1–0 line ratio (R₂₁/₁₀) in the barred spiral galaxy ...
We present the first statistical survey of the properties of the 12CO(1-0) and 12CO(3-2) line emissi...
The CO-to-H2 conversion factor (α CO) is critical to studying molecular gas and star formation in ga...
Carbon monoxide (CO) provides crucial information about the molecular gas properties of galaxies. Wh...
While molecular gas mass is usually derived from (CO)-C-12(J = 1-0)-the most fundamental line for ex...
We present the results of 12CO(J = 1–0) and 13CO(J = 1–0) simultaneous mappings toward the nearby ba...
The correlation between the CO and far infrared luminosities of spiral galaxies is well established....
We present 12CO $J=1$–0 and $J=2$–1 Swedish-ESO Submillimetre Telescope (SEST) observations of the b...
We measure the radial profile of the ^(12)CO(1-0) to H_2 conversion factor (X_(CO)) in NGC 628. The ...
Multi-line studies of CO-12, CO-13, C-18O, HCN, and HCO(+) at 3 mm, 1.3 mm, and 0.8 mm using the Ins...
We estimated physical conditions of molecular gas in the central molecular zone (CMZ) of the Galaxy,...
The CO-to-H2 conversion factor (αCO) is central to measuring the amount and properties of molecular ...
We measure the velocity dispersion, sigma, and surface density, Sigma, of the molecular gas in nearb...
We used the Atacama Pathfinder Experiment (APEX) 12 m telescope to observe the J(KAKc) = 3(03) -> 2(...
Aims. While the search for molecular gas in distant galaxies is based on the detection of submillime...
We present spatial variations of the CO J = 2−1/1–0 line ratio (R₂₁/₁₀) in the barred spiral galaxy ...
We present the first statistical survey of the properties of the 12CO(1-0) and 12CO(3-2) line emissi...
The CO-to-H2 conversion factor (α CO) is critical to studying molecular gas and star formation in ga...
Carbon monoxide (CO) provides crucial information about the molecular gas properties of galaxies. Wh...
While molecular gas mass is usually derived from (CO)-C-12(J = 1-0)-the most fundamental line for ex...
We present the results of 12CO(J = 1–0) and 13CO(J = 1–0) simultaneous mappings toward the nearby ba...
The correlation between the CO and far infrared luminosities of spiral galaxies is well established....
We present 12CO $J=1$–0 and $J=2$–1 Swedish-ESO Submillimetre Telescope (SEST) observations of the b...
We measure the radial profile of the ^(12)CO(1-0) to H_2 conversion factor (X_(CO)) in NGC 628. The ...